scholarly journals Chance, necessity and the origins of life: a physical sciences perspective

Author(s):  
Robert M. Hazen

Earth's 4.5-billion-year history has witnessed a complex sequence of high-probability chemical and physical processes, as well as ‘frozen accidents’. Most models of life's origins similarly invoke a sequence of chemical reactions and molecular self-assemblies in which both necessity and chance play important roles. Recent research adds two important insights into this discussion. First, in the context of chemical reactions, chance versus necessity is an inherently false dichotomy—a range of probabilities exists for many natural events. Second, given the combinatorial richness of early Earth's chemical and physical environments, events in molecular evolution that are unlikely at limited laboratory scales of space and time may, nevertheless, be inevitable on an Earth-like planet at time scales of a billion years. This article is part of the themed issue ‘Reconceptualizing the origins of life’.

2020 ◽  
Vol 498 (1) ◽  
pp. 430-463 ◽  
Author(s):  
Kartheik G Iyer ◽  
Sandro Tacchella ◽  
Shy Genel ◽  
Christopher C Hayward ◽  
Lars Hernquist ◽  
...  

ABSTRACT Understanding the variability of galaxy star formation histories (SFHs) across a range of time-scales provides insight into the underlying physical processes that regulate star formation within galaxies. We compile the SFHs of galaxies at z = 0 from an extensive set of models, ranging from cosmological hydrodynamical simulations (Illustris, IllustrisTNG, Mufasa, Simba, EAGLE), zoom simulations (FIRE-2, g14, and Marvel/Justice League), semi-analytic models (Santa Cruz SAM) and empirical models (UniverseMachine), and quantify the variability of these SFHs on different time-scales using the power spectral density (PSD) formalism. We find that the PSDs are well described by broken power laws, and variability on long time-scales (≳1 Gyr) accounts for most of the power in galaxy SFHs. Most hydrodynamical models show increased variability on shorter time-scales (≲300 Myr) with decreasing stellar mass. Quenching can induce ∼0.4−1 dex of additional power on time-scales >1 Gyr. The dark matter accretion histories of galaxies have remarkably self-similar PSDs and are coherent with the in situ star formation on time-scales >3 Gyr. There is considerable diversity among the different models in their (i) power due to star formation rate variability at a given time-scale, (ii) amount of correlation with adjacent time-scales (PSD slope), (iii) evolution of median PSDs with stellar mass, and (iv) presence and locations of breaks in the PSDs. The PSD framework is a useful space to study the SFHs of galaxies since model predictions vary widely. Observational constraints in this space will help constrain the relative strengths of the physical processes responsible for this variability.


Radiocarbon ◽  
2011 ◽  
Vol 53 (4) ◽  
pp. 691-704 ◽  
Author(s):  
John Southon

Conventional radiocarbon calculations correct for isotopic fractionation using an assumed value of 2.0 for the fractionation of 14C relative to 13C. In other words, isotopic discrimination in physical and chemical processes is assumed to cause relative shifts in 14C/12C ratios that are exactly double those of 13C/12C. This paper analyzes a 1984 experiment that produced a value for the fractionation ratio in photosynthesis of 2.3, which is used to this day by some researchers in the fields of hydrology and speleothem geochemistry. While the value of 2.3 is almost certainly incorrect, theoretical work suggests that the true value may indeed deviate from 2.0, which would have significant implications for 14C calculations.


2016 ◽  
Vol 113 (24) ◽  
pp. E3322-E3331 ◽  
Author(s):  
George Cooper ◽  
Andro C. Rios

Biological polymers such as nucleic acids and proteins are constructed of only one—the d or l—of the two possible nonsuperimposable mirror images (enantiomers) of selected organic compounds. However, before the advent of life, it is generally assumed that chemical reactions produced 50:50 (racemic) mixtures of enantiomers, as evidenced by common abiotic laboratory syntheses. Carbonaceous meteorites contain clues to prebiotic chemistry because they preserve a record of some of the Solar System’s earliest (∼4.5 Gy) chemical and physical processes. In multiple carbonaceous meteorites, we show that both rare and common sugar monoacids (aldonic acids) contain significant excesses of the d enantiomer, whereas other (comparable) sugar acids and sugar alcohols are racemic. Although the proposed origins of such excesses are still tentative, the findings imply that meteoritic compounds and/or the processes that operated on meteoritic precursors may have played an ancient role in the enantiomer composition of life’s carbohydrate-related biopolymers.


1984 ◽  
Vol 24 (01) ◽  
pp. 75-86 ◽  
Author(s):  
R.L. Braun ◽  
J.C. Diaz ◽  
A.E. Lewis

Abstract Lawrence Livermore Natl. Laboratory (LLNL) has developed a one-dimensional (1D) mathematical model to simulate modified in-situ (MIS) retorting of oil shale. In this paper we discuss application of the model to commercial-scale retorting conditions. The model was tested by comparing calculated values to those measured in experimental retort runs performed at LLNL. There was generally good agreement between the calculated and observed results for oil yield, temperature profiles, and the yields of most gas species. Retorting rates were generally overestimated by as much as 10%. The model is a useful tool for design and control of retort operations and to identify and interpret observations that differ from model predictions. The model was used to predict the results for MIS retorting on a commercial scale, focusing on larger retorts and larger shale particle sizes, focusing on larger retorts and larger shale particle sizes than could be investigated experimentally. Retort bed properties, particularly shale composition and particle size, play an important role in determining the recoverable fraction of oil. For a given shale composition, the inlet-gas properties can be selected to help control retort operations and to maximize oil yield. Extreme variations in oil shale grade that may be encountered as a function of depth can be dealt with by appropriate changes in the composition and flow rate of the inlet gas. In addition, we show that substituting oxygen diluted with steam or CO2 (for air or air diluted with steam) can make significant improvements in the heating value of the effluent gas. Finally, we demonstrate the feasibility of retorting through a substantial interval of very low-grade shale. Introduction LLNL has been developing technology applicable to the MIS process of extracting oil from oil shale.1,2 Our program has involved the experimental measurement of chemical reactions and reaction kinetics,3 the operation of pilot-scale retorts,4 and the development of a mathematical model of an MIS retort.5 The objective is to help establish the technical base required to evaluate and apply the MIS method on a commercial scale. A keystone of our program is the retort model, since it represents our cumulative knowledge of the chemical and physical processes involved in oil shale retorting. The retort model has been used in planning and interpreting pilot-scale retort experiments and has successfully predicted most of the results of those experiments.4 It has also been used in developing an operating strategy for a field MIS oil shale retorting experiment.6 The principal purpose of this work is to apply the retort model to a wide range of conditions for MIS retorting, focusing on larger retorts and larger shale particle sizes than can be investigated in a laboratory experiment. Before the results of those calculations are presented, the model is discussed in terms of its content and validity. Model Description The LLNL retort model is a transient, 1D treatment of a packed-bed retort. In developing the model, we adopted a mechanistic approach based on fundamental chemical and physical properties rather than empirical scaling of pilot retort experiments. The model contains no arbitrarily adjustable parameters. A complete mathematical description of the model has been given elsewhere.5 The important features, therefore, are reviewed here only briefly. Our model includes those processes believed to have the most important effects in either the hot-gas retorting mode or the forward combustion mode. The physical processes are axial convective transport of heat and mass, axial thermal dispersion, gas/solid heat transfer, intraparticle shale thermal conductivity, water vaporization and condensation, and wall heat loss. The chemical reactions within the shale particles are the release of bound water, pyrolysis of kerogen, coking of oil, pyrolysis of char, decomposition of carbonate materials, and gasification of residual organic carbon with CO2, H2O, and O2. The chemical reactions in the bulk-gas stream are the combustion and cracking of oil vapor, combustion of H2, CH4, CHx, and CO, and the water/gas shift. The model permits axial variations of initial shale composition, particle-size distribution, and bed void fraction. It also permits time-dependent variations of the composition, flow rate, and temperature of inlet gas. The governing equations for mass and energy balance are solved numerically by a semi-implicit, finite-difference method. The results of these calculations determine the oil yield, and the composition and temperature of both the gas stream and the shale particles as a function of time and location in the retort.


2012 ◽  
Vol 30 (2) ◽  
pp. 357-369 ◽  
Author(s):  
V. M. Vasyliūnas

Abstract. The conventional equations of ionospheric electrodynamics, highly succesful in modeling observed phenomena on sufficiently long time scales, can be derived rigorously from the complete plasma and Maxwell's equations, provided that appropriate limits and approximations are assumed. Under the assumption that a quasi-steady-state equilibrium (neglecting local dynamical terms and considering only slow time variations of external or aeronomic-process origin) exists, the conventional equations specify how the various quantities must be related numerically. Questions about how the quantities are related causally or how the stress equilibrium is established and on what time scales are not anwered by the conventional equations but require the complete plasma and Maxwell's equations, and these lead to a picture of the underlying physical processes that can be rather different from the commonly presented intuitive or ad hoc explanations. Particular instances include the nature of the ionospheric electric current, the relation between electric field and plasma bulk flow, and the interrelationships among various quantities of neutral-wind dynamo.


2018 ◽  
Vol 25 (5) ◽  
pp. 1277-1290 ◽  
Author(s):  
Christian G. Schroer ◽  
Ilya Agapov ◽  
Werner Brefeld ◽  
Reinhard Brinkmann ◽  
Yong-Chul Chae ◽  
...  

The PETRA IV project aims at upgrading the present synchrotron radiation source PETRA III at DESY into an ultralow-emittance source. Being diffraction limited up to X-rays of about 10 keV, PETRA IV will be ideal for three-dimensional X-ray microscopy of biological, chemical and physical processes under realistic conditions at length scales from atomic dimensions to millimetres and time scales down to the sub-nanosecond regime. In this way, it will enable groundbreaking studies in many fields of science and industry, such as health, energy, earth and environment, mobility and information technology. The science case is reviewed and the current state of the conceptual design is summarized, discussing a reference lattice, a hybrid multi-bend achromat with an interleaved sextupole configuration based on the ESRF-EBS design, in more detail as well as alternative lattice concepts.


2013 ◽  
Vol 70 (4) ◽  
pp. 1071-1083 ◽  
Author(s):  
Gilles Bellon ◽  
Bjorn Stevens

Abstract The adjustment of the trade wind atmospheric boundary layer to an abrupt sea surface warming is investigated using a large-eddy simulation (LES) and two simple bulk models: a mixed-layer model (MLM), and a model based on the mixing-line hypothesis (XLM). The near-surface temperature adjusts in a few hours, faster than can be expected from the characteristic time scales associated with the physical processes at play. The near-surface humidity adjusts more slowly, with a time scale of about a day, and it exhibits an initial decrease before increasing to its equilibrium value. An analysis of the MLM suggests that the initial tendency of humidity and temperature results from the difference in Bowen ratios between the equilibrium and the perturbation. An analysis of the three linear modes of the XLM shows that the fastest-decaying mode adjusts the subcloud-layer buoyancy, with a constructive interaction of all of the physical processes. The second-fastest-decaying mode is an adjustment of the boundary layer thermodynamical structure and the slowest mode adjusts the boundary layer depth. Approximate analytical expressions of the time scales characterizing these linear modes are derived both for the MLM and the XLM. The MLM exhibits no scale separation between the fastest and second-fastest time scales and a scale separation between these and the slowest time scale only in the case of a shallow well-mixed boundary layer. The XLM exhibits a scale separation between the buoyancy adjustment of the subcloud layer and the overall thermodynamic adjustment, while conserving the scale separation with the slower adjustment of the boundary layer depth.


2007 ◽  
Vol 46 (8) ◽  
pp. 2413-2422 ◽  
Author(s):  
Changdo Jung ◽  
Sadhan C. Jana ◽  
I. Sedat Gunes

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